HD114762
HIP64426 in T.Bensby+,AAP, 562, A71, 2014
taken from 13 paper(s):
/T.V.Mishenina et al.(2002)/
/T.V.Mishenina and V. V. Kovtyukh(2001)/
/J.P.Fulbright(2000)/
/J.Simmerer et al.(2004)/
/R.G.Gratton et al.(2003)/
/R.Smiljanic et al.(2009)/
/Y.Saito et al.(2009)/
/T.Gehren et al.(2006)/
/B.E.Reddy et al.(2006)/
/T.Bensby et al.(2014)/
/K.A.Venn et al.(2004)/
/P.E.Nissen and W. J. Schuster(2010)/
/P. E. Nissen and W. J. Schuster(2011)/

T.V.Mishenina et al.,AAP, 396, 189, 2002 (A0070,ADS)
Abundances of Cu and Zn in metal-poor stars: Clues for Galaxy evolution
Stellar Parameters
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Fe | N/A | -0.74 | ... | ... | -0.74 | ... | 6.76 | Fe |
Cu I | N/A | ... | -0.06+-0.13 | ... | -0.78+-0.13 | -0.04+-0.13 | 3.41+-0.13 | Cu I |
Zn I | N/A | ... | 0.09+-0.11 | ... | -0.61+-0.11 | 0.13+-0.11 | 3.95+-0.11 | Zn I |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | ELODIE | 42000 | >100 | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
T.V.Mishenina et al.,AAP, 370, 951, 2001 (A0071,ADS)
Analysis of neutron capture elements in metal-poor stars
Stellar Parameters
Teff : 5800 | log g : 4.0 | vturb : 1.0 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Mg I | N/A | ... | 0.17 | ... | -0.57 | 0.15 | 7.03 | Mg I |
Si I | N/A | ... | 0.19 | ... | -0.49 | 0.23 | 7.02 | Si I |
Ca I | N/A | ... | 0.29 | ... | -0.41 | 0.31 | 5.93 | Ca I |
Fe | N/A | -0.72 | ... | ... | -0.72 | ... | 6.78 | Fe |
Sr I | N/A | ... | -0.10 | ... | -0.72 | -0.00 | 2.15 | Sr I |
Ba II | N/A | ... | 0.04 | ... | -0.73 | -0.01 | 1.45 | Ba II |
La II | N/A | ... | -0.01 | ... | -0.66 | 0.06 | 0.44 | La II |
Ce II | N/A | ... | -0.18 | ... | -0.90 | -0.18 | 0.68 | Ce II |
Nd II | N/A | ... | -0.04 | ... | -0.68 | 0.04 | 0.74 | Nd II |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | ELODIE | 42000 | >100 | N/A | N/A |
J.P.Fulbright et al.,AJ, 120, 1841, 2000 (A0126,ADS)
ABUNDANCES AND KINEMATICS OF FIELD HALO AND DISK STARS. I. OBSERVATIONAL DATA AND ABUNDANCE ANALYSIS
Stellar Parameters
Teff : 5800 | log g : 4.1 | vturb : 1.25 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Li I | N/A | ... | ... | 1.99 | -1.27 | -0.47 | 1.99 | Li I |
Na I | N/A | ... | 0.17 | ... | -0.56 | 0.24 | 5.68 | Na I |
Mg I | N/A | ... | 0.43 | ... | -0.41 | 0.39 | 7.19 | Mg I |
Al I | N/A | ... | 0.24 | ... | -0.56 | 0.24 | 5.89 | Al I |
Si I | N/A | ... | 0.32 | ... | -0.46 | 0.34 | 7.05 | Si I |
Ca I | N/A | ... | 0.2 | ... | -0.60 | 0.20 | 5.74 | Ca I |
Ti | N/A | ... | 0.24 | ... | -0.54 | 0.26 | 4.41 | Ti |
V I | N/A | ... | 0.11 | ... | -0.64 | 0.16 | 3.29 | V I |
Cr I | N/A | ... | 0.01 | ... | -0.78 | 0.02 | 4.86 | Cr I |
Fe | N/A | -0.82 | ... | ... | -0.80 | ... | 6.70 | Fe |
Ni I | N/A | ... | 0.05 | ... | -0.74 | 0.06 | 5.48 | Ni I |
Y II | N/A | ... | -0.14 | ... | -0.93 | -0.13 | 1.28 | Y II |
Zr II | N/A | ... | 0.03 | ... | -0.77 | 0.03 | 1.81 | Zr II |
Ba II | N/A | ... | -0.02 | ... | -0.89 | -0.09 | 1.29 | Ba II |
Eu II | N/A | ... | 0.26 | ... | -0.57 | 0.23 | -0.05 | Eu II |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1999-05-24 | N/A | LICKHAMILTON | 50000 | 145 | 600 | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
J.Simmerer et al.,ApJ, 617, 1091, 2004 (A0131,ADS)
The Rise of the s-Process in the Galaxy
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Fe I | N/A | -0.75 | ... | ... | -0.75 | ... | 6.75 | Fe I |
Fe II | N/A | -0.8 | ... | ... | -0.80 | ... | 6.70 | Fe II |
La II | N/A | ... | ... | 0.2 | -0.90 | -0.15 | 0.2 | La II |
Eu II | N/A | ... | ... | -0.24 | -0.76 | -0.01 | -0.24 | Eu II |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | MCDONALD | 60000 | 100 | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
R.G.Gratton et al.,AAP, 404, 187, 2003 (A0135,ADS)
Abundances for metal-poor stars with accurate parallaxes
Stellar Parameters
Teff : 5875 | log g : 4.14 | vturb : 1.2 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Na I | N/A | ... | 0.16+-0.054 | ... | -0.66+-0.054 | 0.14+-0.054 | 5.58+-0.054 | Na I |
Mg I | N/A | ... | 0.47+-0.055 | ... | -0.49+-0.055 | 0.31+-0.055 | 7.11+-0.055 | Mg I |
Si I | N/A | ... | 0.26+-0.048 | ... | -0.51+-0.048 | 0.29+-0.048 | 7.00+-0.048 | Si I |
Ca I | N/A | ... | 0.23+-0.033 | ... | -0.63+-0.033 | 0.17+-0.033 | 5.71+-0.033 | Ca I |
Ti I | N/A | ... | 0.16+-0.03 | ... | -0.51+-0.03 | 0.29+-0.03 | 4.44+-0.03 | Ti I |
Ti II | N/A | ... | 0.17+-0.048 | ... | -0.50+-0.048 | 0.30+-0.048 | 4.45+-0.048 | Ti II |
Fe I | N/A | -0.79+-0.051 | ... | ... | -0.80+-0.051 | ... | 6.70+-0.051 | Fe I |
Fe II | N/A | -0.85+-0.066 | ... | ... | -0.86+-0.066 | ... | 6.64+-0.066 | Fe II |
Binary Parameters
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | N/A | 50000 | >100 | N/A | 49.9 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : 173101 | Right Ascension : 131220 |
R.Smiljanic et al.,AAP, 499, 103, 2009 (A0190,ADS)
Beryllium abundances and star formation in the halo and in the thick disk
Stellar Parameters
Teff : 5800 | log g : 4.1 | vturb : 1.25 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Li | N/A | ... | ... | 2.01 | -1.25 | -0.55 | 2.01 | Li |
Be | N/A | ... | ... | 0.69 | -0.69 | 0.01 | 0.69 | Be |
Fe | N/A | -0.7 | ... | ... | -0.70 | ... | 6.80 | Fe |
Observing Log
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
Y.Saito et al.,PASJ, 61, 549, 2009 (A0208,ADS)
Chemical Evolution of Zinc in the Galaxy
Stellar Parameters
Teff : 5791 | log g : 4.08 | vturb : 1.40 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Fe I | N/A | -0.86 | ... | ... | -0.91 | ... | 6.59 | Fe I |
Fe II | N/A | -0.82 | ... | ... | -0.87 | ... | 6.63 | Fe II |
Zn I | N/A | ... | 0.02+-0.11 | ... | -0.80+-0.11 | 0.11+-0.11 | 3.76+-0.11 | Zn I |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | OAO | 50000 | 160 | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
T.Gehren et al.,AAP, 451, 1065, 2006 (A0259,ADS)
Na, Mg and Al abundances as a population discriminant for nearby metal-poor stars
Stellar Parameters
Teff : 5890 | log g : 4.14+-0.10 | vturb : 1.3 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Na I | 6 | ... | 0.17 | ... | -0.44 | 0.25 | 5.80 | Na I |
Mg I | 7 | ... | 0.21 | ... | -0.51 | 0.18 | 7.09 | Mg I |
Al I | 1 | ... | 0.06 | ... | -0.62 | 0.07 | 5.83 | Al I |
Fe | N/A | -0.70 | ... | ... | -0.69 | ... | 6.81 | Fe |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | FOCES | 40000 | 200 | 4200 | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : +173101.7 | Right Ascension : 131220.10 |
B.E.Reddy et al.,MNRAS, 367, 1329, 2006 (C0002,ADS)
Elemental abundance survey of the Galactic thick disc
Stellar Parameters
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
C | N/A | ... | 0.31 | ... | -0.32 | 0.44 | 8.11 | C |
O | N/A | ... | 0.57 | ... | -0.10 | 0.66 | 8.59 | O |
Na | N/A | ... | 0.06 | ... | -0.62 | 0.14 | 5.62 | Na |
Mg | N/A | ... | 0.33 | ... | -0.44 | 0.32 | 7.16 | Mg |
Al | N/A | ... | 0.16 | ... | -0.72 | 0.04 | 5.73 | Al |
Si | N/A | ... | 0.14 | ... | -0.46 | 0.30 | 7.05 | Si |
Ca | N/A | ... | 0.2 | ... | -0.52 | 0.24 | 5.82 | Ca |
Sc | N/A | ... | 0.05 | ... | -0.57 | 0.19 | 2.58 | Sc |
Ti | N/A | ... | 0.14 | ... | -0.62 | 0.14 | 4.33 | Ti |
V | N/A | ... | -0.01 | ... | -0.65 | 0.11 | 3.28 | V |
Cr | N/A | ... | -0.09 | ... | -0.76 | -0.00 | 4.88 | Cr |
Mn | N/A | ... | -0.36 | ... | -1.13 | -0.37 | 4.30 | Mn |
Fe I | N/A | -0.71 | ... | ... | -0.76 | ... | 6.74 | Fe I |
Co | N/A | ... | 0.09 | ... | -0.68 | 0.08 | 4.31 | Co |
Ni | N/A | ... | -0.04 | ... | -0.74 | 0.02 | 5.48 | Ni |
Cu | N/A | ... | -0.08 | ... | -0.79 | -0.03 | 3.40 | Cu |
Zn | N/A | ... | 0.04 | ... | -0.76 | -0.00 | 3.80 | Zn |
Y | N/A | ... | -0.07 | ... | -0.87 | -0.11 | 1.34 | Y |
Ba | N/A | ... | -0.21 | ... | -0.90 | -0.14 | 1.28 | Ba |
Ce | N/A | ... | 0.09 | ... | -0.62 | 0.14 | 0.96 | Ce |
Nd | N/A | ... | 0.21 | ... | -0.42 | 0.34 | 1.00 | Nd |
Eu | N/A | ... | 0.21 | ... | -0.41 | 0.35 | 0.11 | Eu |
Binary Parameters
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2004-06 | N/A | MCDONALD | 60000 | 100-200 | N/A | 49.4 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
T.Bensby et al.,AAP, 562, A71, 2014 (C0007,ADS)
Exploring the Milky Way stellar disk. A detailed elemental abundance study of 714 F and G dwarf stars in the solar neighbourhood
Stellar Parameters
Teff : 5996+-59 | log g : 4.28+-0.09 | vturb : 1.19+-0.10 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
O | 3 | ... | 0.36+-0.13 | ... | ... | ... | O |
Na | 4 | ... | 0.10+-0.02 | ... | ... | ... | Na |
Mg | 5 | ... | 0.27+-0.04 | ... | ... | ... | Mg |
Al | 7 | ... | 0.21+-0.04 | ... | ... | ... | Al |
Si | 29 | ... | 0.15+-0.03 | ... | ... | ... | Si |
Ca | 17 | ... | 0.18+-0.05 | ... | ... | ... | Ca |
Ti | 27 | -0.50+-0.06 | 0.20+-0.06 | ... | ... | Ti |
Cr | 15 | ... | -0.04+-0.07 | ... | ... | ... | Cr |
Fe | 206 | -0.70+-0.05 | ... | ... | ... | ... | Fe |
Fe I | 185 | ... | ... | 6.86 | ... | ... | Fe I |
Fe II | 21 | ... | ... | 6.85 | ... | ... | Fe II |
Ni | 44 | ... | -0.03+-0.05 | ... | ... | ... | Ni |
Zn | 3 | ... | 0.08+-0.10 | ... | ... | ... | Zn |
Y | 5 | ... | -0.17+-0.16 | ... | ... | ... | Y |
Ba | 3 | ... | -0.16+-0.12 | ... | ... | ... | Ba |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2006-04-01 | N/A | MIKELCO | 65000 | 250 | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
K.A.Venn et al.,AJ, 128, 1177, 2004 (C0011,ADS)
Stellar Chemical Signatures and Hierarchical Galaxy Formation
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Na | N/A | ... | 0.17 | ... | ... | ... | Na |
Mg | N/A | ... | 0.43 | ... | ... | ... | Mg |
Ca | N/A | ... | 0.2 | ... | ... | ... | Ca |
Ti | N/A | ... | 0.24 | ... | ... | ... | Ti |
Fe | N/A | -0.82 | ... | ... | ... | ... | Fe |
Ni | N/A | ... | 0.05 | ... | ... | ... | Ni |
Y | N/A | ... | -0.14 | ... | ... | ... | Y |
Ba | N/A | ... | -0.02 | ... | ... | ... | Ba |
Eu | N/A | ... | 0.26 | ... | ... | ... | Eu |
Observing Log
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : +173102 | Right Ascension : 131219.7 |
P.E.Nissen et al.,AAP, 511, L10, 2010 (C0012,ADS)
Two distinct halo populations in the solar neighborhood. Evidence from stellar abundance ratios and kinematics
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Fe | N/A | -0.70 | ... | ... | -0.70 | ... | 6.80 | Fe |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2006-06-08-0109 | N/A | VLT | 55000 | 475 | N/A | 49.1 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
P. E. Nissen et al.,AAP, 530, A15, 2011 (C0013,ADS)
Two distinct halo populations in the solar neighborhood II. Evidence from stellar abundances of Mn, Cu, Zn, Y, and Ba
Stellar Parameters
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Fe | N/A | -0.7 | ... | ... | -0.70 | ... | 6.80 | Fe |
Zn | N/A | ... | 0.1 | ... | -0.56 | 0.14 | 4.00 | Zn |
Y | N/A | ... | -0.16 | ... | -0.83 | -0.13 | 1.38 | Y |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2006-06-08-0109 | N/A | VLT | 55000 | 475 | N/A | 49.1 |